Solar Images Thursday, 13 October 2022

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Photosphere sunspot drawing and RDS evaluation

13.10.2022 photosphere drawing

High-resolution scan (3231 px)

Time
07:25 UT
Observer
Burçin TANIK
g
5
f
22
R
72
Seeing
3 / 5

Sunspot groups and observation details →

Sunspot groups (from the drawing)

RDS data file (.gzd)
[Gözlem]
Tarih=13.10.2022
Saat=07:25
Gözlemci=Burçin TANIK
KontrolEden=Olcay PLEVNE
Durumaçısı=26.23
Enlemaçısı=6.02
Boylamaçısı=335.41
Boylamfark=3
GKalite=3
GDurum=G.T , B.A , K.T
Kuzeyaçısı=-0.2
Sırano=19574
AyRasatNo=9
RasatÖnceki=12.10.2022
RasatSonraki=14.10.2022

[Leke Grupları]
Grupsayısı=5:4:1
LekeSayısı=22:21:1
RölatifSayı=72:61:11
01=HH_ 01 +29.297 +70.670 046.800 +0.000 0000 0 +30.364 +72.700 +28.230 +68.640 +29.297 +72.200 +29.297 +69.140
02=ESI 06 +20.850 +70.430 045.453 +0.000 0000 0 +25.970 +76.799 +15.720 +63.287 +20.850 +76.599 +20.850 +63.487
03=DAC 11 +28.583 +31.942 007.352 22.299 0000 0 +30.612 +36.517 +26.554 +27.367 +26.760 +35.258 +29.742 +27.960
04=BXI 03 +23.135 -65.343 270.670 23.445 0000 0 +24.850 -60.997 +21.421 -69.690 +21.856 -62.481 +24.641 -68.922
05=AX_ 01 -28.159 -48.558 286.852 -1.000 0000 0 -28.159 -48.558 -28.159 -48.558
20221013.gzd

Chromosphere (H-α) FITS frames

H-α

The images are made automatically with a fixed, gentle rule: uneven illumination and most of the limb darkening are removed, and the brightness is shown on a linear scale (no sharpening); prominences get their own scale outside the limb. Frames are ordered by sharpness (seeing); frames without the Sun (darks, bias) come last. Method →

2022/20221013_bto · BTO · 1 frames · 21.4 MB · 07:41:24 UT

Coronado H-α animations from frame sequences

No Coronado observation for this day.